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Hydrodynamic stability and stellar oscillations

โœ Scribed by H M ANTIA

Book ID
107588988
Publisher
Springer-Verlag
Year
2011
Tongue
English
Weight
447 KB
Volume
77
Category
Article
ISSN
0304-4289

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This paper discusses the hydrodynamic modeling offlarmg plasma confined in magnetic loops and its objectives within the broader scope of flare physics. In particular, the Palermo-Harvard model is discussed along with its applications to the detailed fitting of X-ray light curves of solar flares and